[Ne II] velocity maps for sources with spatially extended [Ne II] emission. In each of the three categories, the sources are ordered by increasing disk inclination (read from left to right and top to bottom). The velocities (in each pixel and v_c) are corrected for stellar radial velocity and disk inclination. Only pixels with flux greater than 2σ are shown, where σ is the standard deviation of the background calculated iteratively. The red star in each map marks the centroid of the corresponding continuum, and the white horizontal line passing through it highlights the known disk PA (Table 1). Sources with asterisks are further discussed in Appendix D. The highly inclined disks (incl. > 80°) are indicated by highlighting their v_c in magenta, and their maps (as well as v_c) are not deprojected for inclination. The [Ne II] jetlike velocity maps show broader emission than expected for jets; however, this is a PSF effect, and deconvolution reveals [Ne II] jets that are narrower than H₂ winds (e.g., SY Cha; K. R. Schwarz et al. 2025). The [Ne II] spectra toward each source in this figure and the corresponding Gaussian fits to estimate v_c are shown in Appendix B.